Artículo

El editor solo permite decargar el artículo en su versión post-print desde el repositorio. Por favor, si usted posee dicha versión, enviela a
Consulte el artículo en la página del editor
Consulte la política de Acceso Abierto del editor

Abstract:

We examine an interacting dark matter variable vacuum energy model for a spatially flat Friedmann-Roberston-Walker spacetime, focusing on the appearance of cosmological singularities such as big rip, big brake, big freeze, and big separation along with abrupt events (infinite γ- singularity and new w-singularity) at late times. We introduce a phenomenological interaction which has a nonlinear dependence on the total energy density of the dark sector and its derivative, solve exactly the source equation for the model and find the energy density as a function of the scale factor as well as the time dependence of the approximate scale factor in the neighborhood of the singularities. We describe the main characteristics of these singularities by exploring the type of interaction that makes them possible along with behavior of dark components near them. We apply the geometric Tipler and Królak method for determining the fate of timelike geodesic curves around the singularities. We also explore the strength of them by analyzing the leading term in some geometric invariants such as the square Riemann scalar and the Ricci scalar. © 2015 American Physical Society.

Registro:

Documento: Artículo
Título:Interacting realization of cosmological singularities with variable vacuum energy
Autor:Chimento, L.P.; Richarte, M.G.
Filiación:Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires and IFIBA, CONICET, Ciudad Universitaria, Pabellón I, Buenos Aires, 1428, Argentina
Departamento de Física, Facultad de Ciencias Exactas y Naturales, Universidad de Buenos Aires, Ciudad Universitaria, Pabellón I, Buenos Aires, 1428, Argentina
Año:2015
Volumen:92
Número:4
DOI: http://dx.doi.org/10.1103/PhysRevD.92.043511
Título revista:Physical Review D - Particles, Fields, Gravitation and Cosmology
Título revista abreviado:Phys Rev D Part Fields Gravit Cosmol
ISSN:15507998
CODEN:PRVDA
Registro:https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_15507998_v92_n4_p_Chimento

Referencias:

  • Wang, Y., (2010) Dark Energy, , (Wiley, New York)
  • Wang, Y., (2010) Dark Energy: Observational and Theoretical Approaches, , edited by P. Ruiz-Lapuente (Cambridge University Press, Cambridge)
  • Ade P, A.R., (2014) Astron. Astrophys., 571, p. A16
  • Hinshaw, G., (2013) Astrophys. J. Suppl. Ser., 208, p. 19
  • Barrow J, D., Galloway, G., Tipler, F., (1986) Mon. Not. R. Astron. Soc., 223, p. 835
  • Caldwell, R.R., (2002) Phys. Lett. B, 545, p. 23
  • Starobinsky, A.A., (2000) Gravitation Cosmol., 6, p. 157
  • Chimento L, P., Lazkoz, R., (2003) Phys. Rev. Lett., 91, p. 211301
  • Dabrowski M, P., Stachowiak, T., Szydlowski, M., (2003) Phys. Rev. D, 68, p. 103519
  • González-Díaz P, F., (2004) Phys. Rev. D, 69, p. 063522
  • Nojiri, S.I., Odintsov S, D., (2004) Phys. Rev. D, 70, p. 103522
  • Balcerzak, A., Dabrowski M, P., (2006) Phys. Rev. D, 73, p. 101301
  • Nojiri, S.I., Odintsov S, D., Tsujikawa, S., (2005) Phys. Rev. D, 71, p. 063004
  • Gorini, V., Kamenshchik A, Y., Moschella, U., Pasquier, V., (2004) Phys. Rev. D, 69, p. 123512
  • Keresztes, Z., Gergely L, A., Kamenshchik A, Y., (2012) Phys. Rev. D, 86, p. 063522
  • Barrow, D.J., (2004) Classical Quantum Gravity, 21, p. L79
  • Barrow J, D., Tsagas C, G., (2005) Classical Quantum Gravity, 22, p. 1563
  • Nojiri, S., Odintsov S, D., (2005) Phys. Rev. D, 72, p. 023003
  • Yu Kamenshchik, A., (2013) Classical Quantum Gravity, 30, p. 173001
  • Bouhmadi-López, M., González-Díaz P, F., Martín-Moruno, P., (2008) Phys. Lett. B, 659, p. 1
  • Bouhmadi-López, M., González-Díaz P, F., Martín-Moruno, P., (2008) Int. J. Mod. Phys. D, 17, p. 2269
  • Bouhmadi-López, M., Kiefer, C., Sandhofer, B., Moniz P, V., arXiv:1002.4783; Nojiri, S., Odintsov S, D., (2008) Phys. Rev. D, 78, p. 046006
  • Bamba, K., Nojiri, S., Odintsov S, D., J. Cosmol. Astropart. Phys., 2008 (10), p. 045
  • Lip, Z.W.S., (2011) Phys. Rev. D, 83, p. 023528
  • Hawking S, W., Ellis G, F.R., (1973) The Large Scale Structure of Spacetime, , (Cambridge University Press, Cambridge)
  • Fernandez-Jambrina, L., Lazkoz, R., (2006) Phys. Rev. D, 74, p. 064030
  • Fernandez-Jambrina, L., Lazkoz, R., (2004) Phys. Rev. D, 70, p. 121503
  • Barrow J, D., Cotsakis, S., (2013) Phys. Rev. D, 88, p. 067301
  • Tipler, J.F., (1977) Phys. Lett., 64 A, p. 8
  • Krolak, A., (1986) Classical Quantum Gravity, 3, p. 267
  • Clarke C, J.S., Krolak, A., (1985) J. Geom. Phys., 2, p. 127
  • Królak, A., Rudnicki, W., (1993) Int. J. Theor. Phys., 32, p. 137
  • Chimento, P.L., (2010) Phys. Rev. D, 81, p. 043525
  • Chimento L, P., Richarte M, G., (2011) Phys. Rev. D, 84, p. 123507
  • Chimento L, P., Richarte M, G., (2012) Phys. Rev. D, 85, p. 127301
  • Chimento L, P., Richarte M, G., (2012) Phys. Rev. D, 86, p. 103501
  • Chimento L, P., Richarte M, G., (2013) Eur. Phys. J. C, 73, p. 2352
  • Chimento L, P., Richarte M, G., (2013) Eur. Phys. J. C, 73, p. 2497
  • Chimento L, P., Richarte M, G., García, E.S.I., (2013) Phys. Rev. D, 88, p. 087301
  • Chimento, P.L., (2004) Phys. Rev. D, 69, p. 123517
  • Barrow, D.J., (1990) Phys. Lett. B, 235, p. 40
  • Dabrowski M, P., Denkieiwcz, T., (2009) Phys. Rev. D, 79, p. 063521
  • Bouhmadi-Lopez, M., Chen, P., Liu, Y.-W., (2013) Eur. Phys. J. C, 73, p. 2546
  • Fernández-Jambrina, L., (2014) Phys. Rev. D, 90, p. 064014
  • Ruzmaikina, T., Ruzmaikin A, A., (1970) Sov. Phys. JETP, 30, p. 372
  • Stefancic, H., (2005) Phys. Rev. D, 71, p. 084024
  • Bouhmadi-López, M., (2008) Nucl. Phys., B797, p. 78
  • Fernández-Jambrina, L., (2010) Phys. Rev. D, 82, p. 124004
  • A FRW spacetime, curves of the form (Equation presented) with (Equation presented) being the proper time fulfil the geodesic equation, (Equation presented), provided the only component of 4-velocity is (Equation presented), (Equation presented), and (Equation presented); For a FRW metric, the squared Riemann is given by (Equation presented) and the Ricci scalar is (Equation presented); The weak energy condition corresponds to the case with (Equation presented) and (Equation presented); the null condition only involves the latter inequality ((Equation presented)) whereas the strong energy condition is satisfied if (Equation presented) and (Equation presented); Barrow J, D., Graham A, H., (2015) Phys. Rev. D, 91, p. 083513
  • Nojiri, S., Odintsov S, D., Oikonomou, V.K., (2015) Phys. Rev. D, 91, p. 084059
  • S. Nojiri, S.D. Odintsov, V.K. Oikonomou, and Emmanuel N. Saridakis, arXiv:1503.08443; Nojiri, S., Odintsov S, D., Oikonomou, V.K., (2015) Phys. Lett. B, 747, p. 310

Citas:

---------- APA ----------
Chimento, L.P. & Richarte, M.G. (2015) . Interacting realization of cosmological singularities with variable vacuum energy. Physical Review D - Particles, Fields, Gravitation and Cosmology, 92(4).
http://dx.doi.org/10.1103/PhysRevD.92.043511
---------- CHICAGO ----------
Chimento, L.P., Richarte, M.G. "Interacting realization of cosmological singularities with variable vacuum energy" . Physical Review D - Particles, Fields, Gravitation and Cosmology 92, no. 4 (2015).
http://dx.doi.org/10.1103/PhysRevD.92.043511
---------- MLA ----------
Chimento, L.P., Richarte, M.G. "Interacting realization of cosmological singularities with variable vacuum energy" . Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 92, no. 4, 2015.
http://dx.doi.org/10.1103/PhysRevD.92.043511
---------- VANCOUVER ----------
Chimento, L.P., Richarte, M.G. Interacting realization of cosmological singularities with variable vacuum energy. Phys Rev D Part Fields Gravit Cosmol. 2015;92(4).
http://dx.doi.org/10.1103/PhysRevD.92.043511